Infrared spectropolarimetry of Seyfert galaxy NGC 1068

Details Infrared spectropolarimetry of Seyfert galaxy NGC 1068 Infrared spectropolarimetry of Seyfert galaxy NGC 1068

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.310..660a&link_type=abstract

Nature (ISSN 0028-0836), vol. 310, Aug. 23, 1984, p. 660-662.

Astronomy and Astrophysics

Astronomy

26

Galactic Nuclei, Infrared Astronomy, Infrared Spectra, Polarimetry, Seyfert Galaxies, Emission Spectra, Far Infrared Radiation, Interstellar Matter, Polarization Characteristics, Radiant Flux Density

Scientific paper

Spectropolarimetric measurements of NGC 1068 between 8 and 13 microns are presented which show that the polarized flux at these wavelengths is intrinsic to the emission mechanism and is not due to absorption by aligned grains. Data on the flux, polarization, position angle, and polarized intensity are presented and their implications for various published models are discussed.

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